Relation between $γ$-rays and emission lines for the $γ$-ray loud blazars
| dc.creator | Fan, J. H. | |
| dc.date | 2000-07-21 | |
| dc.date.accessioned | 2026-07-07T01:54:29Z | |
| dc.date.available | 2026-07-07T01:54:29Z | |
| dc.description | The relation between the $γ$-ray and the emission line luminosities for a sample of 36 $γ$-ray loud blazars is investigated; an apparent correlation between them, $L_γ \propto L_{Line}^{0.69\pm0.11}$, with a correlation coefficient $r=0.741$ and a chance probability of $p = 1.9\times10^{-6}$, is found. It is found, however, that there is no intrinsic correlation between them: the apparent correlation is due to the redshift dependence in a flux-limited sample. Thus no evidence is found to support the argument that the up-scattered soft photons are from the broad emission lines. Our analysis does not conflict with the SSC model. The disk-jet symbiosis and radio/$γ$-ray correlation found in the literature are also discussed. The radio/$γ$-ray correlation may be an apparent correlation caused by the boosting effect since both bands are strongly beamed. | |
| dc.description | 1 table, 2 figures, 4 pages, in A&A, 358, 841-844 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0007326 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0007326 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1372 | |
| dc.subject | Astrophysics | |
| dc.title | Relation between $γ$-rays and emission lines for the $γ$-ray loud blazars | |
| dc.type | text |